Thursday, December 14, 2023

NASA's Johnson Space Center: The Year 2023 in Review

NASA's Johnson Space Center: The Year 2023 in Review


Highlights of the year 2023 at NASA's Johnson Space Center in Houston, Texas. 

Learn more about Johnson Space Center: 

The Johnson Space Center (JSC) was established in 1961 as the Manned Spacecraft Center, the home and Mission Control Center for the U.S. human space flight program. In 1973, it was renamed in honor of the late President, and Texas native, Lyndon B. Johnson.

Video Credit: NASA's Johnson Space Center (JSC)
Duration: 3 minutes, 39 seconds
Release Date: Dec. 13, 2023


#NASA #Space #Astronomy #Science #JWST #Earth #ISS #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #Mars #DeepSpace #MoonToMars #Engineering #SpaceTechnology #SpaceExploration #SolarSystem #HumanSpaceflight #JSC #Houston #Texas #UnitedStates #STEM #Education #HD #Video

Wednesday, December 13, 2023

NASA’s Perseverance Rover Deciphers Ancient History of Martian Lake | JPL

NASA’s Perseverance Rover Deciphers Ancient History of Martian Lake | JPL

This 360-degree mosaic from the “Airey Hill” location inside Jezero Crater was generated using 993 individual images taken by the Perseverance Mars rover’s Mastcam-Z from Nov. 3-6. The rover remained parked at Airey Hill for several weeks during solar conjunction.
This image of Mars’ Jezero Crater is overlaid with mineral data detected from orbit by NASA's Mars Reconnaissance Orbiter (MRO). The green color represents carbonatesminerals that form in watery environments with conditions that might be favorable for preserving signs of ancient life. NASA’s Perseverance is currently exploring the green area above Jezero’s fan (center).

Now at 1,000 days on Mars, the mission has traversed an ancient river and lake system, collecting valuable samples along the way.

Marking its 1,000th Martian day on the Red Planet, NASA’s Perseverance rover recently completed its exploration of the ancient river delta that holds evidence of a lake that filled Jezero Crater billions of years ago. The six-wheeled scientist has to date collected a total of 23 samples, revealing the geologic history of this region of Mars in the process.

One sample called “Lefroy Bay” contains a large quantity of fine-grained silica, a material known to preserve ancient fossils on Earth. Another, “Otis Peak,” holds a significant amount of phosphate. This is often associated with life as we know it. Both of these samples are also rich in carbonate, which can preserve a record of the environmental conditions from when the rock was formed.

The discoveries were shared Tuesday, Dec. 12, 2023, at the American Geophysical Union (AGU) fall meeting in San Francisco.

“We picked Jezero Crater as a landing site because orbital imagery showed a delta—clear evidence that a large lake once filled the crater. A lake is a potentially habitable environment, and delta rocks are a great environment for entombing signs of ancient life as fossils in the geologic record,” said Perseverance’s project scientist, Ken Farley of Caltech. “After thorough exploration, we’ve pieced together the crater’s geologic history, charting its lake and river phase from beginning to end.”

Jezero formed from an asteroid impact almost 4 billion years ago. After Perseverance landed in February 2021, the mission team discovered the crater floor is made of igneous rock formed from magma underground or from volcanic activity at the surface. They have since found sandstone and mudstone, signaling the arrival of the first river in the crater hundreds of millions of years later. Above these rocks are salt-rich mudstones, signaling the presence of a shallow lake experiencing evaporation. The team thinks the lake eventually grew as wide as 22 miles (35 kilometers) in diameter and as deep as 100 feet (30 meters).

Later, fast-flowing water carried in boulders from outside Jezero, distributing them atop of the delta and elsewhere in the crater.

“We were able to see a broad outline of these chapters in Jezero’s history in orbital images, but it required getting up close with Perseverance to really understand the timeline in detail,” said Libby Ives, a postdoctoral fellow at NASA’s Jet Propulsion Laboratory (JPL) in Southern California that manages the mission.

Enticing Samples

The samples Perseverance gathers are about as big as a piece of classroom chalk and are stored in special metal tubes as part of the Mars Sample Return campaign, a joint effort by NASA and the European Space Agency (ESA). Bringing the tubes to Earth would enable scientists to study the samples with powerful lab equipment too large to take to Mars.

To decide which samples to collect, Perseverance first uses an abrasion tool to wear away a patch of a prospective rock and then studies the rock’s chemistry using precision science instruments, including the JPL-built Planetary Instrument for X-ray Lithochemistry, or PIXL.

At a target the team calls “Bills Bay,” PIXL spotted carbonates—minerals that form in watery environments with conditions that might be favorable for preserving organic molecules. (Organic molecules form by both geological and biological processes.) These rocks were also abundant with silica, a material that is excellent at preserving organic molecules, including those related to life.

“On Earth, this fine-grained silica is what you often find in a location that was once sandy,” said JPL’s Morgan Cable, the deputy principal investigator of PIXL. “It’s the kind of environment where, on Earth, the remains of ancient life could be preserved and found later.”

Perseverance’s instruments are capable of detecting both microscopic, fossil-like structures and chemical changes that may have been left by ancient microbes, but they have yet to see evidence for either.

At another target PIXL examined, called “Ouzel Falls,” the instrument detected the presence of iron associated with phosphate. Phosphate is a component of DNA and the cell membranes of all known terrestrial life and is part of a molecule that helps cells carry energy.

After assessing PIXL’s findings on each of these abrasion patches, the team sent up commands for the rover to collect rock cores close by: Lefroy Bay was collected next to Bills Bay, and Otis Peak at Ouzel Falls.

“We have ideal conditions for finding signs of ancient life where we find carbonates and phosphates, which point to a watery, habitable environment, as well as silica, which is great at preservation,” Cable said.

Perseverance’s work is, of course, far from done. The mission’s ongoing fourth science campaign will explore Jezero Crater’s margin, near the canyon entrance where a river once flooded the crater floor. Rich carbonate deposits have been spotted along the margin, which stands out in orbital images like a ring within a bathtub.

More About the Mission

A key objective for Perseverance’s mission on Mars is astrobiology, including the search for signs of ancient microbial life. The rover will characterize the planet’s geology and past climate, pave the way for human exploration of the Red Planet, and be the first mission to collect and cache Martian rock and regolith (broken rock and dust).

Subsequent NASA missions, in cooperation with the European Space Agency, would send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.

The Mars 2020 Perseverance mission is part of NASA’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.

JPL, which is managed for NASA by Caltech in Pasadena, California, built and manages operations of the Perseverance rover.

For more about Perseverance:

mars.nasa.gov/mars2020/


Credit: NASA/JPL-Caltech/ASU/MSSS

Release Date: Dec. 12, 2023


#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #Mars2020 #PerseveranceRover #JezeroCrater #AncientLake #MarsSampleReturn #MSR #Robotics #SpaceTechnology #Engineering #JPL #Caltech #UnitedStates #STEM #Education

Recientemente: Las primeras imágenes enviadas por nuestra nave espacial Psyche

Recientemente: Las primeras imágenes enviadas por nuestra nave espacial Psyche


FriendsofNASA.org: Recientemente en la NASA, la versión en español de las cápsulas This Week at NASA, te informa semanalmente de lo que está sucediendo en la NASA. 

Ciencia de la NASA: https://ciencia.nasa.gov

Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: https://www.nasa.gov/suscribete


Credit: National Aeronautics and Space Administration (NASA)

Duration: 2 minutes, 48 seconds

Release Date: Dec. 12, 2023


#NASA #Space #ISS #ISS25 #Earth #NASAenespañol #español #ClimateChange #GlobalWarming #Science #Astronauts #Europe #JAXA #Canada #Japan #Cosmonauts #Russia #HumanSpaceflight #Expedition70 #History #PsycheMission #Asteroids #STEM #Education #HD #Video

Ax-3 Mission Overview | Axiom Space | International Space Station

Ax-3 Mission Overview | Axiom Space | International Space Station

Axiom Space held a virtual press conference with leaders from NASA and SpaceX, as well as leaders from the Italian Air Force, the Turkish Space Agency (TUA), and the European Space Agency (ESA) to provide a high-level review of mission operations and objectives to officially kick off major media efforts leading up to Axiom Mission 3 (Ax-3).

Ax-3 will be the first all-European commercial astronaut mission to launch to the ISS—redefining the pathway to low-Earth orbit (LEO) and helping chart a course toward Axiom Station, the world’s first commercial space station.

As part of Ax-3, Türkiye is sending its first astronaut to space in a larger effort to expand the nation’s space exploration capabilities and establish a national human spaceflight program. Ax-3 will also be the first commercial spaceflight mission for an ESA-sponsored astronaut. For Italy, the Ax-3 mission represents a whole-of-country effort to expand its access to space for the purposes of research, development, and innovation. 

The Ax-3 crewmembers are Commander Michael López-Alegría of the U.S. and Spain, Pilot Walter Villadei of the Italian Air Force, and Mission Specialists Alper Gezeravcı of Türkiye and Marcus Wandt of Sweden and ESA. A SpaceX Falcon 9 rocket will launch the Ax-3 crew aboard a Dragon spacecraft to the International Space Station (ISS) no earlier than January 2024 from NASA’s Kennedy Space Center in Florida.

"Axiom Space is guided by the vision of a thriving home in space that benefits every human, everywhere. The leader in providing space infrastructure as a service, Axiom offers end-to-end missions to the International Space Station today while privately developing its successor – a permanent commercial destination in Earth’s orbit that will sustain human growth off the planet and bring untold benefits back home."

More information about Axiom can be found at www.axiomspace.com

Video Credit: Axiom Space

Duration: 44 minutes

Release Date: Dec. 13, 2023


#NASA #Space #ISS #AxiomSpace #Ax3Mission #Ax3 #AX3Crew #Astronauts #MichaelLópezAlegría #WalterVilladei #AlperGezeravcı #MarcusWandt #SpaceX #CrewDragon #Falcon9Rocket #CommercialSpace #Science #SpaceLaboratory #InternationalCooperation #UnitedStates #ESA #Italy #Türkiye #Sweden #STEM #Education #HD #Video

NASA 2023: "Nothing is Beyond Our Reach"

NASA 2023: "Nothing is Beyond Our Reach"

"NASA’s mission is to explore the unknown in air and space, to innovate for the benefit of humanity, and to inspire the world through discovery." 

"NASA showed the world that anything is possible in 2023."

To learn more about the missions mentioned in this highlight video, take a deep dive into these links:

OSIRIS-REx: https://go.nasa.gov/41h1xWJ

James Webb Space Telescope: https://go.nasa.gov/3uY0u1V

Psyche: https://go.nasa.gov/3uVtcQZ

Nuclear Propulsion: https://go.nasa.gov/3uVtcQZ

International Partnerships: https://go.nasa.gov/47UUKV2 (PDF)

Earth Observations: https://earthobservatory.nasa.gov/

Earth Information Center: https://go.nasa.gov/3Rc1GG8

Sustainable Flight Demonstrator: https://go.nasa.gov/46WqY0Q

International Space Station 25 Years in Low Earth Orbit: https://youtu.be/zY2Zn1cKExY

Frank Rubio Record: https://go.nasa.gov/41nyGjI

International Science Missions: https://go.nasa.gov/3TgZ1he

First Woman Issue #2: https://www.nasa.gov/calliefirst/

NASA+: https://plus.nasa.gov/

Moon to Mars Architecture: https://go.nasa.gov/4ahH7Rl

Artemis III Spacesuit Prototype: https://go.nasa.gov/4719ArL

Space Launch System Hardware Production: https://go.nasa.gov/41hwYQM

RS-25 Tests: https://go.nasa.gov/3RkhF59

Engines Installed: https://go.nasa.gov/47ROoWI

Orion Production: https://go.nasa.gov/41jHxCK

Artemis II Crew Announced: https://go.nasa.gov/3Rc20EQ


Video Credit: National Aeronautics and Space Administration (NASA)

Duration: 3 minutes

Release Date: Dec. 12, 2023


#NASA #ESA #Space #Astronomy #Science #JWST #Earth #ISS #Moon #ArtemisProgram #ArtemisII #OrionSpacecraft #Mars #DeepSpace #MoonToMars #Engineering #SpaceTechnology #SpaceExploration #HumanSpaceflight #SolarSystem #UnitedStates #Europe #International #STEM #Education #HD #Video

Pan of Star Cluster IC 348 in Perseus | Webb Telescope

Pan of Star Cluster IC 348 in Perseus | Webb Telescope

This image from the near-infrared camera (NIRCam) instrument on the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope shows the central portion of the star cluster IC 348. Astronomers combed the cluster in search of tiny, free-floating brown dwarfs: objects too small to be stars but larger than most planets. They found three brown dwarfs that are less than eight times the mass of Jupiter. The smallest weighs just three to four times as much as Jupiter, challenging theories for star formation.

The wispy curtains filling the image are interstellar material reflecting the light from the cluster’s stars—known as a reflection nebula. The material also includes carbon-containing molecules called polycyclic aromatic hydrocarbons, or PAHs. The bright star closest to the center of the frame is actually a pair of type B stars in a binary system, the most massive stars in the cluster. Winds from these stars may help sculpt the large loop seen on the right side of the field of view.


Credit: NASA, ESA, CSA, STScI, and K. Luhman (Penn State University) and C. Alves de Oliveira (European Space Agency), N. Bartmann (ESA/Webb)

Duration: 30 seconds

Release Date: Dec. 13, 2023


#NASA #Space #Astronomy #Science #Stars #Starclusters #Starcluster #IC348 #BrownDwarfStars #ReflectionNebula #Perseus #Constellation #Galaxy #Cosmos #Universe #JWST #Infrared #SpaceTelescope #ESA #GSFC #STScI #UnitedStates #ESA #CSA #STEM #Education #HD #Video

Star Cluster IC 348: Three Brown Dwarf Stars Identified | Webb Telescope

Star Cluster IC 348: Three Brown Dwarf Stars Identified | Webb Telescope



These images from the near-infrared camera (NIRCam) instrument on the NASA/European Space Agency/Canadian Space Agency James Webb Space Telescope shows the central portion of the star cluster IC 348. Astronomers combed the cluster in search of tiny, free-floating brown dwarfs: objects too small to be stars but larger than most planets. They found three brown dwarfs that are less than eight times the mass of Jupiter. The smallest weighs just three to four times as much as Jupiter, challenging theories for star formation.

The wispy curtains filling the image are interstellar material reflecting the light from the cluster’s stars—what is known as a reflection nebula. The material also includes carbon-containing molecules known as polycyclic aromatic hydrocarbons, or PAHs. The bright star closest to the center of the frame is actually a pair of type B stars in a binary system, the most massive stars in the cluster. Winds from these stars may help sculpt the large loop seen on the right side of the field of view.

Image 1 Description: Wispy hair-like filaments of pink-purple fill the middle of the image, curving left and right on either side of the center. On the right, the filaments form a dramatic loop that seems to extend toward the viewer. At lower left are additional yellowish filaments. Two prominent, bright stars near the center of the image show Webb’s eight-point diffraction spikes. Dozens of fainter stars are scattered across the image.

Image 2 Description: Image of a star cluster and nebula, with three image details pulled out in square boxes stacked vertically along the right. Main image is showing wispy pink-purple filaments and a scattering of stars. Each of the three boxes along the right corresponds to a small detail, numbered and circled, in the main image. Box 1 (top): A detail from the lower left of the main image shows a pair of small circular pinkish-white spots on a yellowish-brown background. Box 2 (middle): A detail from the middle of the lower part of the main image shows a single small circular pinkish spot on a yellowish-brown background. Box 3: A detail from the lower right edge of the main image shows a small circular pinkish spot on a dark brown background.


Credit: NASA, ESA, CSA, STScI, and K. Luhman (Penn State University) and C. Alves de Oliveira (European Space Agency)

Release Date: Dec. 13, 2023


#NASA #Space #Astronomy #Science #Stars #Starclusters #Starcluster #IC348 #BrownDwarfStars #ReflectionNebula #Perseus #Constellation #Galaxy #Cosmos #Universe #JWST #Infrared #SpaceTelescope #ESA #GSFC #STScI #UnitedStates #ESA #CSA #STEM #Education

Tuesday, December 12, 2023

Fireball! | Geminid Meteor over Colorado

Fireball! | Geminid Meteor over Colorado

Every December we have a chance to see one of our favorite meteor showers—the Geminids. All meteors appear to come from the same place in the sky called the radiant. The Geminids appear to radiate from a point in the constellation Gemini, hence the name “Geminids.”

The Geminids are typically rich in green-colored fireballs like this one!

The Geminids are caused by debris from a celestial object known as 3200 Phaethon, whose origin is the subject of debate. A number of astronomers consider it to be an extinct comet, based on observations showing a small amount of material leaving Phaethon’s surface. Others argue that it has to be an asteroid because of its orbit and its similarity to the main-belt asteroid Pallas.

Whatever the nature of Phaethon, observations show that the Geminids are denser than meteors belonging to other showers, enabling them to get as low as 29 miles above Earth’s surface before burning up. Meteors belonging to other showers, like the Perseids, burn up much higher.

The Geminids can be seen by most of the world. Yet, it is best viewed by observers in the Northern Hemisphere. As you enter the Southern Hemisphere and move towards the South Pole, the altitude of the Geminid radiant—the celestial point in the sky where the Geminid meteors appear to originate—gets lower and lower above the horizon. Thus, observers in these locations see fewer Geminids than their northern counterparts.

Besides the weather, the phase of the Moon is a major factor in determining whether a meteor shower will have good rates during any given year.

Meteors can be colorful. While the human eye usually cannot discern many colors, cameras often can. Colors in meteors usually originate from ionized chemical elements released as the meteor disintegrates. Blue-green colors typically originate from magnesium, calcium radiates violet, and nickel glows green. Red, however, typically originates from energized nitrogen and oxygen in the Earth's atmosphere. This bright meteoric fireball was gone in a flash—less than a second—but it left a wind-blown ionization trail that remained visible.

Learn more about meteors and meteorites:


Image Credit: Mike Lewinski

Location: near Crestone, Colorado, United States

Image Date:  Dec. 11, 2023


#NASA #Space #Astronomy #Science #Planet #Earth #Atmosphere #Meteors #Bolides #Fireballs #Astrophotography #MikeLewinski #Astrophotographer #CitizenScience #SolarSystem #Colorado #UnitedStates #NorthernHemisphere #STEM #Education

Mars: December 2023 Images | NASA Mars Curiosity & Perseverance Rovers | JPL

Mars: December 2023 Images | NASA Mars Curiosity & Perseverance Rovers | JPL

Mars 2020 - sol 995
MSL - sol 4030
MSL - sol 4030
Mars 2020 - sol 997
MSL - sol 4033
MSL - sol 4032
Mars 2020 - sol 996
MSL - sol 4030
   

Celebrating 11+ Years on Mars (2012-2023)
Mission Name: Mars Science Laboratory (MSL)
Rover Name: Curiosity
Main Job: To determine if Mars was ever habitable to microbial life. 
Launch: Nov. 6, 2011
Landing Date: Aug. 5, 2012, Gale Crater, Mars

Celebrating 2+ Years on Mars
Mission Name: Mars 2020
Rover Name: Perseverance
Main Job: Seek signs of ancient life and collect samples of rock and regolith (broken rock and soil) for return to Earth.
Mars Helicopter (Ingenuity)
Launch: July 30, 2020    
Landing: Feb. 18, 2021, Jezero Crater, Mars

For more information on NASA's Mars missions, visit: mars.nasa.gov

Image Credits: NASA/JPL-Caltech/ASU/MSSS
Processing: Kevin M. Gill
Image Release Dates: Dec. 7, 2023

#NASA #Space #Astronomy #Science #Mars #RedPlanet #Planet #Astrobiology #Geology #CuriosityRover #MSL #MountSharp #GaleCrater #PerseveranceRover #Mars2020 #JezeroCrater #Robotics #SpaceTechnology #SpaceEngineering #JPL #Caltech #UnitedStates #CitizenScience #KevinGill #STEM #Education

Espacio a Tierra - Encendiendo el futuro - 8 de diciembre de 2023

Espacio a Tierra - Encendiendo el futuro - 8 de diciembre de 2023

Espacio a Tierra, la versión en español de las cápsulas Space to Ground de la NASA, te informa semanalmente de lo que está sucediendo en la Estación Espacial Internacional. 

Ciencia de la NASA: https://ciencia.nasa.gov

Para obtener más información sobre la ciencia de la NASA, suscríbete al boletín semanal: https://www.nasa.gov/suscribete


Credit: NASA's Johnson Space Center (JSC)

Duration: 3 minutes, 31 seconds

Release Date: Dec. 12, 2023


#NASA #Space #ISS #ISS25 #Earth #NASAenespañol #español #Science #Astronauts #LoralOHara #JasminMoghbeli #UnitedStates #AndreasMogensen #Denmark #Danmark #Europe #SatoshiFurukawa #JAXA #Japan #日本 #Cosmonauts #Russia #HumanSpaceflight #Expedition70 #History #STEM #Education #HD #Video

Pan: Cluster in the Cloud Globular Cluster NGC 2210 | Hubble

Pan: Cluster in the Cloud Globular Cluster NGC 2210 | Hubble

This striking image shows the densely packed globular cluster known as NGC 2210. It is situated in the Large Magellanic Cloud (LMC). The LMC lies about 157,000 light-years from Earth. It is a so-called satellite galaxy of the Milky Way, meaning that the two galaxies are gravitationally bound. Globular clusters are very stable, tightly bound clusters of thousands or even millions of stars. Their stability means that they can last a long time, and therefore globular clusters are often studied in order to investigate potentially very old stellar populations. 

In fact, 2017 research that made use of this data used to build this image revealed that a sample of LMC globular clusters were incredibly close in age to the oldest stellar clusters found in the Milky Way’s halo. They found that NGC 2210 is around 11.6 billion years old. Although this is only a couple of billion years younger than the Universe itself, it makes NGC 2210 by far the youngest globular cluster in their sample. All other LMC globular clusters studied in the same work were found to be older, with four of them over 13 billion years old. This is interesting, because it tells astronomers that the oldest globular clusters in the LMC formed contemporaneously with the oldest clusters in the Milky Way, although the two galaxies formed independently. 

As well as being a source of interesting research, this old-but-relatively-young cluster is also extremely beautiful with its highly concentrated population of stars. The night sky would look very different from the perspective of an inhabitant of a planet orbiting one of the stars in a globular cluster’s center. The sky would appear to be stuffed full of stars, in a stellar environment that is thousands of times more crowded than our own.

Image Description: A dense cluster of stars. It is brightest and most crowded in the center, where the stars are mostly a cool white color. Moving out towards the edges the stars become more spread out and reddish until a noticeable ‘edge’ to the cluster is reached. Beyond that edge there are still many stars, more disorganized and seen on a black background. A number of stars appear to be in front of the cluster.

Science paper in the Monthly Notices of the Royal Astronomical Society: 

https://academic.oup.com/mnras/article/471/3/3347/3930867


Credit: ESA/Hubble & NASA, A. Sarajedini, F. Niederhofer

Duration: 30 seconds

Release Date: Dec. 10, 2023


#NASA #ESA #Astronomy #Hubble #Space #Science #Stars #GlobularClusters #GlobularCluster #NGC2210 #Dorado #Constellation #Galaxies #LargeMagellanicCloud #LMC #Cosmos #Universe #HubbleSpaceTelescope #HST #GSFC #STScI #UnitedStates #Europe #STEM #Education #HD #Video

The "Squid Galaxy": M77 in Cetus | Schulman Telescope

The "Squid Galaxy": M77 in Cetus | Schulman Telescope

Located 47 million light-years away in the constellation of Cetus (The Sea Monster), barred spiral galaxy Messier 77 is one of the most remote galaxies of the Messier catalogue. Messier 77 (M77) is also known as NGC 1068 or the Squid Galaxy. 

Messier 77 was discovered by French astronomer Pierre Méchain in 1780, who originally described it as a nebula. Méchain then communicated his discovery to his counterpart Charles Messier, who subsequently listed the object in his astronomical catalog. Messier and German-British astronomer William Herschel described this galaxy as a star cluster. Today, however, with modern technology, the object is known to be a galaxy.

At approximately 100,000 light-years across, Messier 77 is also one of largest galaxies in the Messier catalogue—so massive that its gravity causes other nearby galaxies to twist and become warped.

Technical Details

Optics: Schulman 32-inch RCOS Telescope

Camera: SBIG STX16803

The 0.81 m (32 in) Schulman Telescope is a Ritchey-Chrétien reflector built by RC Optical Systems and installed in 2010. It is operated by the Mount Lemmon SkyCenter and is Arizona's largest dedicated public observatory. The Schulman Telescope was designed from inception for remote control over the Internet by amateur and professional astrophotographers worldwide. It is currently the world's largest telescope dedicated for this purpose.


Image Credit & Copyright: Adam Block/Mount Lemmon SkyCenter/University of Arizona

Caption Acknowledgements: European Southern Observatory (ESO)/Wikipedia

Image Date: Nov. 1, 2014


#NASA #Astronomy #Space #Science #Galaxies #Galaxy #Messier77 #NGC1068 #BarredGalaxy #SpiralGalaxy #TypeIISeyfertGalaxy #AGNGalaxy #Cetus #Cosmos #Universe #UA #MountLemmonObservatory #SchulmanTelescope #Astrophotographer #AdamBlock #Arizona #UnitedStates #STEM #Education

Tribute to NASA Astronaut Kathryn Thornton | Hubble Servicing Mission#1

Tribute to NASA Astronaut Kathryn Thornton | Hubble Servicing Mission#1









STS-61 was NASA's first Hubble Space Telescope servicing mission, and the fifth flight of the Space Shuttle Endeavour. On her third spaceflight, Dr. Kathryn Thornton was a mission specialist extravehicular activity (EVA) crew member aboard the Space Shuttle Endeavour on the STS61 Hubble Space Telescope (HST) servicing and repair mission. STS-61 launched at night from the Kennedy Space Center, Florida, on December 2, 1993. 

During the 11-day flight, the HST was captured and restored to full capacity through a record five space walks by four astronauts. After having traveled 4,433,772 miles in 163 orbits of the Earth, the crew of Endeavour returned to a night landing at the Kennedy Space Center on December 13, 1993.

Astronaut Kathryn Thornton Official NASA Biography:

Image Credit: NASA's Johnson Space Center (JSC)
Image Dates: Jan. 23, 1990 - Dec. 8, 1993

#NASA #ESA #Astronomy #Space #Science #Hubble #HubbleServicingMission1 #Astronaut #KathrynThornton #Astronauts #SpaceShuttle #SpaceShuttleEndeavour #STS61 #Universe #HST #HubbleSpaceTelescope #GSFC #STScI #UnitedStates #Europe #History #STEM #Education

Monday, December 11, 2023

China's iSpace Hyperbola-2 Commercial Rocket: Vertical Takeoff & Landing Test

China's iSpace Hyperbola-2 Commercial Rocket: Vertical Takeoff & Landing Test


iSpace’s Hyperbola-2 (双曲线二号, SQX-2) launch vehicle performed a second successful vertical takeoff, vertical landing (VTVL) test at the Jiuquan Satellite Launch Center, China, on December 10, 2023, at 09:07 UTC (17:07 local time). Hyperbola-2 is a small, reusable, two-stage liquid-propellant launch vehicle, designed by iSpace (星际荣耀, Beijing Interstellar Glory Space Technology Corporation Ltd) to launch up to 1.9 tons on a low-Earth orbit. 

This second successful hop test “marks a major breakthrough in China’s commercial aerospace industry in reusable launch vehicle technology. It also signals the charge for China’s aerospace sector to catch up with the world’s most advanced levels in reusable launch vehicle technology” an iSpace statement read.

The test is part of the company’s plan to develop the Hyperbola-3 rocket with a reusable first stage. iSpace is skipping the previously-planned smaller Hyperbola-2, the company stated at the 9th China (International) Commercial Aerospace Forum in July 2023.

The company is targeting a first flight of the 13.4-metric-ton to low Earth orbit (LEO) Hyperbola-3 rocket in 2025. A demonstration of reuse will follow in 2026. The 69-meter-long rocket will be able to lift 8.5 tons to LEO in reusable mode. iSpace says it aims to conduct 25 Hyperbola-3 launches per year by 2030.

The Hyperbola-3B, a triple-core version of the rocket, akin to the Falcon Heavy in configuration, will be capable of carrying no less than 15 tons to LEO, according to iSpace.

iSpace made history as the first privately-funded Chinese company to reach orbit in 2019 with the solid-fueled Hyperbola-1 rocket. The company however suffered three consecutive failures with the rocket, before a successful return to flight earlier this year. Further launches of the solid rocket are expected in the coming year, despite competition from Galactic Energy’s Ceres-1 and Expace’s Kuaizhou rockets.

iSpace is not the only Chinese company working on reusable rockets. Galactic Energy recently performed a hop test with a jet engine-powered article. CAS Space, a spin-off from the Chinese Academy of Sciences, has likewise conducted such tests to verify algorithms. Deep Blue Aerospace completed a successful kilometer-level rocket launch and landing test in 2022.

Another competitor, Space Pioneer, is planning to launch its Tianlong-3 rocket in the first half of 2024. The rocket will be comparable to Falcon 9 in launch capability and eventually to be made reusable. Landspace’s methalox Zhuque-2 is also expected to be converted for reusability.

China opened up its space sector to private and commercial activity in 2014. This is seen as largely in reaction to the explosion of commercial space in the U.S. The central government has since implemented policies and published guidance to support the development of commercial space.

2023 has been a notable year for China’s commercial launch companies. CAS Space, Galactic Energy, iSpace, Expace, Space Pioneer and Landspace have all reached orbit. These include first Chinese commercial liquid propellant launch successes, achieved by Space Pioneer and Landspace.

The Tiangong Space Station is expected to provide an opportunity for commercial launch vehicles to gain contracts to deliver cargo. The national Guowang LEO broadband megaconstellation is also expected to provide opportunities for commercial actors.


Video Credit: iSpace (Beijing Interstellar Glory Space Technology Corporation Ltd)/China Central Television (CCTV)/China Global Television Network (CGTN)

Acknowledgements: SciNews

Duration: 2 minutes, 31 seconds

Release Date: Dec. 11, 2023


#NASA #Space #China #中国 #iSpace #星际荣耀 #Hyperbola2 #SQX2 #双曲线二号 #Rocket #VTVL #MethaneLiquidOxygen #CH4LOX #LEO #Spaceflight #JiuquanSatelliteLaunchCenter #JSLC #GansuProvince #CommercialSpace #Satellites #TiangongSpaceStation #ChinaSpaceStation #CSS #STEM #Education #HD #Video

Planet Mars: The Day the Solar Wind Disappeared | NASA Goddard

Planet Mars: The Day the Solar Wind Disappeared | NASA Goddard

In December 2022, NASA’s Mars-orbiting MAVEN mission observed the dramatic and unexpected “disappearance” of the solar wind, a stream of charged particles that continuously emanates from the Sun. This was caused by a special type of solar event that was so powerful, it created a void in its wake as it traveled through the solar system. The Martian atmosphere and magnetosphere expanded by thousands of kilometers in response, causing the solar wind to temporarily vanish from Mars. MAVEN’s observations of this dramatic event are helping scientists to better understand the physics that drive atmospheric and water loss at Mars.

 Learn more about MAVEN at: https://science.nasa.gov/mission/maven


Credit: NASA’s Goddard Space Flight Center (GSFC)

Kel Elkins: Lead Data Visualizer

Dan Gallagher: Producer/Narrator

Greg Shirah: Data Visualizer

Cindy Starr: Data Visualizer

Walt Feimer: Animator

John Blackwell: Animator

Jonathan North: Animator

Chris Meaney: Animator

Jasper Halekas: Scientist

Skylar Shaver: Scientist

Abigail Azari: Scientist

Yingjuan Ma: Scientist

Shannon Curry: Scientist

Willow Reed: Communications

Nancy Neal-Jones: Public Affairs

Duration: 2 minutes, 46 seconds

Release Date: Dec. 11, 2023


#NASA #Space #Astronomy #Science #Planet #Mars #Atmosphere #Star #Sun #SolarWind #MAVENMission #MAVENSpacecraft #SolarSystem #SpaceExploration #GSFC #LASP #CUBoulder #UnitedStates #STEM #Education #HD #Video

All Lined Up: Interacting Galaxy System Arp-Madore 2105-332 | Hubble

All Lined Up: Interacting Galaxy System Arp-Madore 2105-332 | Hubble


This image features an interacting galaxy system known as Arp-Madore 2105-332, that lies about 200 million light-years from Earth in the constellation Microscopium. This system belongs to the Arp-Madore catalogue of peculiar galaxies. The wonderful quality of this image also reveals several further galaxies, not associated with this system but fortuitously positioned in such a way that they appear to be forming a line that approaches the leftmost (in this image) component of Arp-Madore 2105-332. This is known individually as 2MASX J21080752-3314337. The rightmost galaxy, meanwhile, is known as 2MASX J21080362-3313196. These hefty names do not lend themselves to easy memorization, but they do actually contain valuable information. They are coordinates in the right ascension and declination system used widely by astronomers to locate astronomical objects.

Both the galaxies are of a type known as emission-line galaxies. This simply means that, when observed with spectrometers, the spectra of both galaxies exhibit characteristic bright peaks, known as emission lines. This is distinct from, for example, absorption-line galaxies whose spectra contain distinct gaps, known as absorption lines. Emission lines are produced when gases are very hot, and therefore have sufficient energy that the atoms and molecules are ‘excited’ and emit light. In other words, emission-line galaxies are highly energetic places, marking them out as likely hotbeds of star formation.

As with many galaxy types, categorizing a galaxy as an emission-line galaxy does not exclude it from having other descriptions that refer to its other properties. Arp-Madore 2105-332, for example, is also a ‘peculiar’ galaxy, reflecting the atypical shapes of its two constituent galaxies.

Image Description: A pair of interacting galaxies, one smaller than the other. Each has a bright spot at the center and two loosely-wound spiral arms, with threads of dark dust following the arms. They appear as a broad, soft glow in which individual stars can’t be seen. A number of bright stars and smaller, background galaxies can also be seen — three such galaxies lie in a vertical line below the right-hand galaxy of the pair.


Credit: ESA/Hubble & NASA, J. Dalcanton

Acknowledgement: L. Shatz

Release Date: Dec. 11, 2023


#NASA #ESA #Hubble #Astronomy #Space #Science #Hubble #Galaxies #ArpMadore2105332 #Galaxy #2MASXJ210807523314337 #2MASXJ210803623313196 #EmissionLineGalaxies #PeculiarGalaxies #Microscopium #Constellation #Cosmos #Universe #HST #SpaceTelescope #STScI #GSFC #UnitedStates #Europe #STEM #Education